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20102014
most citedOGLE-2008-BLG-355Lb: A Massive Planet around A Late type Star

23 citations · 23 across the 1 of their papers we have counts for

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10 papers

astro-ph.EP2014★ 23 cited

OGLE-2008-BLG-355Lb: A Massive Planet around A Late type Star

N. Koshimoto, A. Udalski, T. Sumi +32

We report the discovery of a massive planet OGLE-2008-BLG-355Lb. The light curve analysis indicates a planet:host mass ratio of q = 0.0118 +/- 0.0006 at a separation of 0.877 +/- 0…

astro-ph.EP2013

MOA-2008-BLG-379Lb: A Massive Planet from a High Magnification Event with a Faint Source

D. Suzuki, A. Udalski, T. Sumi +31

We report analysis of high microlensing event MOA-2008-BLG-379, which has a strong microlensing anomaly at its peak, due to a massive planet with a mass ratio of q = 6.9 x 10^{-3}.…

astro-ph.SR2013

Microlensing Discovery of a Population of Very Tight, Very Low-mass Binary Brown Dwarfs

J. -Y. Choi, C. Han, A. Udalski +121

Although many models have been proposed, the physical mechanisms responsible for the formation of low-mass brown dwarfs are poorly understood. The multiplicity properties and minim…

astro-ph.EP2013

A Giant Planet beyond the Snow Line in Microlensing Event OGLE-2011-BLG-0251

N. Kains, R. Street, J. -Y. Choi +128

We present the analysis of the gravitational microlensing event OGLE-2011-BLG-0251. This anomalous event was observed by several survey and follow-up collaborations conducting micr…

hep-ex2012

Measurement of forward neutral pion transverse momentum spectra for = 7TeV proton-proton collisions at LHC

O. Adriani, L. Bonechi, M. Bongi +26

The inclusive production rate of neutral pions in the rapidity range greater than has been measured by the Large Hadron Collider forward (LHCf) experiment during LHC $\sqrt…

astro-ph.EP2012

A New Type of Ambiguity in the Planet and Binary Interpretations of Central Perturbations of High-Magnification Gravitational Microlensing Events

J. -Y. Choi, I. -G. Shin, C. Han +118

High-magnification microlensing events provide an important channel to detect planets. Perturbations near the peak of a high-magnification event can be produced either by a planet…